Search for radio emission from the nearby binary brown dwarf system ε Indi Bab

Monthly Notices of the Royal Astronomical Society(2004)

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摘要
We have observed the nearest known brown dwarfs, the binary system ε Indi Bab (d= 3.626 pc), for 8.6- and 4.8-GHz radio emission with the Australia Telescope Compact Array. If either brown dwarf emits radio flares, then they are respectively at least 5.5 and 1.2 times weaker than LP 944-20, the nearest brown dwarf with detected radio emission. We associate the ROSAT source 1WGA J2203.9 − 5647 with...
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关键词
stars: individual: ε Indi Bab,stars: low-mass, brown dwarfs,radio continuum: stars
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